Skip to main content
Log in

Infrared photometry of open clusters: the main sequence of NGC 752

  • Session 1 Stellar Structure and Evolution
  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

New infrared photometry of a sample of 39 stars in the open cluster NGC 752 is presented. These observations confirm the bimodality of the Main Sequence previously reported. We analyze the nature of this behaviour on the basis of the binary hypothesis.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Arribas, S. and Martinez Roger, C.: 1987,Astron. Astrophys. Suppl. Ser. 70, 303.

    Google Scholar 

  • Beckman, J. and Rebolo, R.: 1988, in G. Cayrel de Strobel and M. Spite (eds.),The Impact of Very High S/N Spectroscopy on Stellar Physics, pp. 473–476.

  • Ebbighausen, E. G.: 1939,Astrophys. J. 89, 431.

    Google Scholar 

  • Eggen, O. J.: 1963,Astrophys. J. 138, 356.

    Google Scholar 

  • Johnson, H. L.: 1953,Astrophys. J. 117, 357.

    Google Scholar 

  • Johnson, H. L.: 1966,Ann. Rev. Astron. Astrophys. 4, 193.

    Google Scholar 

  • Twarog, B. A.: 1983,Astrophys. J. 267, 207.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Arribas, S., Manteiga, M., Martinez Roger, C. et al. Infrared photometry of open clusters: the main sequence of NGC 752. Astrophys Space Sci 169, 49–53 (1990). https://doi.org/10.1007/BF00640685

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00640685

Keywords

Navigation